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31.
32.
Modeling path delays in the neutral atmosphere for the analysis of Very Long Baseline Interferometry (VLBI) observations has
been improved significantly in recent years by the use of elevation-dependent mapping functions based on data from numerical
weather models. In this paper, we present a fast way of extracting both, hydrostatic and wet, linear horizontal gradients
for the troposphere from data of the European Centre for Medium-range Weather Forecasts (ECMWF) model, as it is realized at
the Vienna University of Technology on a routine basis for all stations of the International GNSS (Global Navigation Satellite
Systems) Service (IGS) and International VLBI Service for Geodesy and Astrometry (IVS) stations. This approach only uses information
about the refractivity gradients at the site vertical, but no information from the line-of-sight. VLBI analysis of the CONT02
and CONT05 campaigns, as well as all IVS-R1 and IVS-R4 sessions in the first half of 2006, shows that fixing these a priori
gradients improves the repeatability for 74% (40 out of 54) of the VLBI baseline lengths compared to fixing zero or constant
a priori gradients, and improves the repeatability for the majority of baselines compared to estimating 24-h offsets for the
gradients. Only if 6-h offsets are estimated, the baseline length repeatabilities significantly improve, no matter which a
priori gradients are used. 相似文献
33.
Temperature variations at very long baseline interferometry (VLBI) sites cause thermal deformations of the VLBI antennas and
corresponding displacements of the VLBI reference points. The thermal deformation effects typically contain seasonal and daily
signatures. The amplitudes of the annual vertical motion of the antenna reference point can reach several millimeters, depending
on the design of the antenna structure, on the material, and on the environmental effects such as global station position,
station height and climatology effects. Simple methods to correct this effect use the difference of the environmental temperature
with respect to a defined reference temperature, the antenna dimensions, the elevation of the antenna, the material of antenna
structure. Applying these simple models for thermal deformation in the VLBI data analysis improves the baseline length repeatability
by 3.5%. A comparison of these simple models with local thermal deformation measurements at the antennas in Onsala and Wettzell
show that the local measurements and the modeled corrections agree well when the temperature of the antenna structure is used,
but agree less good when the surrounding air temperatures are used. To overcome this problem we present a method to model
temperature penetration into the antenna structures, that allows to model thermal deformation effects that agree with the
observed vertical deformation of the Onsala and Wettzell radio telescopes with a root mean square deviation of 0.07 and 0.13 mm,
respectively. Possible implementations in the VLBI analysis are presented, and the definition of an adequate reference temperature
is discussed. 相似文献
34.
差分VLBI通过交替观测目标天体和参考天体,将共同的误差因素从观测量中扣除,能够实现高精度的相对定位,因而在深空探测中有重要作用。然而,差分VLBI高精度的实现要求目标天体和参考天体的角距很近,这大大限制了其应用。讨论设计了差分VLBI测量的一种实现方案,利用多颗参考源的观测内插出目标源的非几何时延修正,放宽了对目标源和参考源的角距限制。该方案在S波段对目标源非几何时延的修正精度可以达到1 ns水平。 相似文献
35.
空间VLBI的研究现状 总被引:2,自引:0,他引:2
评述了过去近三十年中空间VLBI的发展.其内容包括空间VLBI的简短发展历史,空间VLBI与地面VLBI的不同、空间VLBI的目前状况和空间VLBI的未来展望。着重介绍了作为首次空间VLBI的VSOP的各个方面情况,并给出了VSOP的连续谱、谱线普查样本,供参考。 相似文献
36.
分析了1979年8月至1996年1月之间由MarkⅢVLBI时延资料得到的IAU1980章动模型在经度(δψ)和交角(δε)方向的偏移序列,得到了对IAU1980章动模型中主项系数的改正,并检测了自由地核章动。计算步骤依照常规资料处理方法设计,并采用了一些分析技巧以便充分利用资料的整个时段和减小端部效应对参数解的影响。对拟合残差序列的进一步分析表明,自由地核章动是统计显著的,但其参数尤其是其振幅可能具有时变性质,表现为在经度和交角方向自1986至1995年的持续减弱。 相似文献
37.
MINQUE for block diagonal bordered systems such as those encountered in VLBI data analysis 总被引:1,自引:1,他引:0
A sparse matrix method is developed for computing variance factors for block-diagonal, bordered systems of equations using
MINQUE (Minimum Norm Quadratic Unbiased Estimation). This method greatly reduces the computational effort required to apply
MINQUE, thus making it practical to compute variance factors for some very large systems of equations. The computer implementation
of the method is described and applied to the computation of variance factors for a combination of 1609 VLBI (Very Long Baseline
Interferometry) observing sessions. The purpose of this test was to compute a variance factor for each of the data sets and,
perhaps, to obtain more realistic variance estimates to replace those in common use for the analysis of VLBI data. It was
found that the method is satisfactory for use with such large problems, and the test served to verify that the variances in
current use in VLBI data adjustments are adequate.
Received: 26 November 1996 / Accepted: 12 December 1997 相似文献
38.
39.
40.
2009年11月,云南天文台射电天文研究团组采用40m射电望远镜以及基于DBBC(Digital Base Band Conveter)和Mark5B的VLBI记录系统对PSRJ08354510和PSRJ0332+5434进行了观测。观测选用S波段右旋圆极化信号,起始频率为2206.99MHz,总带宽为32MHz。对数据进行相干消色散和平均后,得到PSRJ0332+5434的单脉冲图像和两颗脉冲星的平均脉冲轮廓。由平均轮廓的展宽随时间的变化关系,对脉冲星的视周期作了一定修正后,得到信噪比更高的平均轮廓图。最后对轮廓的信噪比随时间的变化作了初步分析,由此可了解整个系统在观测时的稳定性。 相似文献